Adams, J.B. & McCord, T.B. (1970) Remote sensing of lunar surface mineralogy: Implications from visible and near-infrared reflectivity of Apollo 11 samples. Proceedings of the Apollo 11 Lunar Sci. Conf., 3, 1937–1945.Google Scholar

Blewett, D.T., Lucey, P.G., Hawke, B.R., & Jolliff, B.L. (1997a) Clementine images of the lunar sample-return stations: Refinement of FeO and TiO₂ mapping techniques. Journal of Geophysical Research, 102, 16319–16325.CrossRefGoogle Scholar

Blewett, D.T., Lucey, P.G., Hawke, B.R., Ling, G.G., & Robinson, M.S. (1997b) A comparison of mercurian reflectance and spectral quantities with those of the Moon. Icarus, 129, 217–231.CrossRefGoogle Scholar

Blewett, D.T., Robinson, M.S., Denevi, B.W., et al. (2009) Multispectral images of Mercury from the first MESSENGER flyby: Analysis of global and regional color trends. Earth and Planetary Science Letters, 285, 272–282.Google Scholar

Blewett, D.T., Chabot, N.L., Denevi, B.W., et al. (2011) Hollows on Mercury: Evidence from MESSENGER for geologically recent volatile-related activity. Science, 333, 1856–1859.Google Scholar

Blewett, D.T., Vaughan, W.V., Xiao, Z., et al. (2013) Mercury’s hollows: Constraints on formation and composition from analysis of geological setting and spectral reflectance. Journal of Geophysical Research, 118, 1013–1032.CrossRefGoogle Scholar

Braden, S.E. & Robinson, M.S. (2013) Relative rates of optical maturation of regolith on Mercury and the Moon. Journal of Geophysical Research, 118, 1903–1914.Google Scholar

Charette, M.P., McCord, T.B., Pieters, C.M., & Adams, J.B. (1974) Application of remote spectral reflectance measurements to lunar geology classification and determination of titanium content of lunar soils. Journal of Geophysical Research, 79, 1605–1613.CrossRefGoogle Scholar

Cloutis, E.A., McCormack, K.A., Bell, J.F., et al. (2008) Ultraviolet spectral reflectance properties of common planetary minerals. Icarus, 197, 321–347.Google Scholar

Cloutis, E.A., Hudon, P., Hiroi, T., Gaffey, M.J., & Mann, P. (2011) Spectral reflectance properties of carbonaceous chondrites: 2. CM chondrites. Icarus, 216, 309–346.Google Scholar

Denevi, B.W. & Robinson, M.S. (2008) Mercury’s albedo from Mariner 10: Implications for the presence of ferrous iron. Icarus, 197, 239–246.Google Scholar

Denevi, B.W., Robinson, M.S., Solomon, S.C., et al. (2009) The evolution of Mercury’s crust: A global perspective from MESSENGER. Science, 324, 613–618.Google Scholar

Denevi, B.W., Ernst, C.M., Meyer, H.M., et al. (2013a) The distribution and origin of smooth plains on Mercury. Journal of Geophysical Research, 118, 891–907.Google Scholar

Denevi, B.W., Ernst, C.M., Whitten, J.L., et al. (2013b) The volcanic origin of a region of intercrater plains on Mercury. 44th Lunar Planet. Sci. Conf., Abstract #1218.Google Scholar

Denevi, B.W., Chabot, N.L., Murchie, S.L., et al. (2018), Calibration, projection, and final image products of MESSENGER’s Mercury Dual Imaging System, Space Science Reviews, 214, 1–52.Google Scholar

Denevi, B.W., Ernst, C.M., Prockter, L.M., & Robinson, M.S. (2019) The geologic history of Mercury. In: Mercury: The view after MESSENGER (Solomon, S.C., Nittler, L.R., & Anderson, B. J., eds.). Cambridge University Press, Cambridge.Google Scholar

Domingue, D.L., Chapman, C.R., Killen, R.M., et al. (2014) Mercury’s weather-beaten surface: Understanding Mercury in the context of lunar and asteroidal space weathering studies. Space Science Reviews, 181, 121–214.Google Scholar

Domingue, D.L., Denevi, B.W., Murchie, S.L., & Hash, C. (2016) Application of multiple photometric models to disk-resolved measurements of Mercury’s surface: Insights into Mercury’s regolith characteristics. Icarus, 268, 172–203.CrossRefGoogle Scholar

Emery, J.P., Sprague, A.L., Witteborn, F.C., Colwell, J.E., Kozlowski, R.W.H., & Wooden, D.H. (1998) Mercury: Thermal modeling and mid-infrared (5–12 µm) observations. Icarus, 136, 104–123.CrossRefGoogle Scholar

Ernst, C.M., Murchie, S.L., Barnouin, O.S., et al. (2010) Exposure of spectrally distinct material by impact craters on Mercury: Implications for global stratigraphy. Icarus, 209, 210–223.Google Scholar

Ernst, C.M., Denevi, B.W., Barnouin, O.S., et al. (2015) Stratigraphy of the Caloris basin, Mercury: Implications for volcanic history and basin impact melt. Icarus, 250, 413–429.Google Scholar

Evans, L.G., Peplowski, P.N., Rhodes, E.A., et al. (2012) Major-element abundances on the surface of Mercury: Results from the MESSENGER Gamma-Ray Spectrometer. Journal of Geophysical Research, 117, E00L07, DOI:10.1029/2012JE004178.Google Scholar

Fassett, C.I., Head, J.W., Baker, D.M.H., et al. (2012) Large impact basins on Mercury: Global distribution, characteristics, and modification history from MESSENGER orbital data. Journal of Geophysical Research, 117, E00L08, DOI:10.1029/2012JE004154.CrossRefGoogle Scholar

Fischer, E.M. & Pieters, C.M. (1994) Remote determination of exposure degree and iron concentration of lunar soils using VIS-NIR spectroscopic methods. Icarus, 111, 475–488.Google Scholar

Gaffey, M.J. (2010) Space weathering and the interpretation of asteroid reflectance spectra. Icarus, 209, 564–574.Google Scholar

Gillis-Davis, J.J., van Niekerk, D., Scott, E.R.D., McCubbin, F.M., & Blewett, D.T. (2013) Impact darkening: A possible mechanism to explain why Mercury is spectrally dark and featureless. Abstract P11A–07, presented at 2013 Fall Meeting, American Geophysical Union, San Francisco, December 9–13.Google Scholar

Goudge, T.A., Head, J.W., Kerber, L., et al. (2014) Global inventory and characterization of pyroclastic deposits on Mercury: New insights into pyroclastic activity from MESSENGER orbital data. Journal of Geophysical Research, 119, 635–658.Google Scholar

Hapke, B. (1977) Interpretations of optical observations of Mercury and the Moon. Physics of the Earth and Planetary Interiors, 15, 264–274.Google Scholar

Hapke, B. (2001) Space weathering from Mercury to the asteroid belt. Journal of Geophysical Research, 106, 10,039–10,073.Google Scholar

Hapke, B., Danielson, G.E., Klaasen, K., & Wilson, L. (1975) Photometric observations of Mercury from Mariner 10. Journal of Geophysical Research, 80, 2431–2443.CrossRefGoogle Scholar

Hawkins, S.E. III, Boldt, J.D., Darlington, E.H., et al. (2007) The Mercury Dual Imaging System on the MESSENGER spacecraft. Space Science Reviews, 131, 247–338.Google Scholar

Head, J.W., Murchie, S.L., Prockter, L.M., et al. (2008) Volcanism on Mercury: Evidence from the first MESSENGER flyby. Science, 321, 69–72.Google Scholar

Head, J.W., Murchie, S.L., Prockter, L.M., et al. (2009) Volcanism on Mercury: Evidence from the first MESSENGER flyby for extrusive and explosive activity and the volcanic origin of plains. Earth and Planetary Science Letters, 285, 227–242.Google Scholar

Head, J.W., Chapman, C.R., Strom, R.G., et al. (2011) Flood volcanism in the high northern latitudes of Mercury revealed by MESSENGER. Science, 333, 1853–1856.Google Scholar

Hendrix, A.R. & Vilas, F. (2006) The effects of space weathering at UV wavelengths: S-class asteroids. Astronomical Journal, 132, 1396–1404.CrossRefGoogle Scholar

Hendrix, A.R., Retherford, K.D., Gladstone, G.R., et al. (2012) The lunar far-UV albedo: Indicator of hydration and weathering. Journal of Geophysical Research, 117, E12001, DOI:10.1029/2012JE004252.Google Scholar

Izenberg, N.R., Klima, R.L., Murchie, S.L., et al. (2014) The low-iron, reduced surface of Mercury as seen in spectral reflectance by MESSENGER. Icarus, 228, 364–374.CrossRefGoogle Scholar

Izenberg, N.R., Thomas, R.J., Blewett, D.T., & Nittler, L.R. (2015) Are there compositionally different types of hollows on Mercury? 46th Lunar Planet. Sci. Conf., Abstract #1344.Google Scholar

Kerber, L., Head, J.W., Blewett, D.T., et al. (2011) The global distribution of pyroclastic deposits on Mercury: The view from MESSENGER flybys 1–3. Planetary and Space Science, 59, 1895–1909.Google Scholar

Klima, R.L., Dyar, M.D., & Pieters, C.M. (2011) Near-infrared spectra of clinopyroxenes: Effects of calcium content and crystal structure. Meteoritics and Planetary Science, 42, 235–253.CrossRefGoogle Scholar

Klima, R.L., Izenberg, N.R., Murchie, S.L., et al. (2013) Constraining the ferrous iron content of minerals in Mercury’s crust. 44th Lunar Planet. Sci. Conf., Abstract #1602.Google Scholar

Klima, R.L., Denevi, B.W., Ernst, C.M., Murchie, S.L., & Peplowski, P.N. (2018) Global distribution and spectral properties of low-reflectance material on Mercury. Geophysical Research Letters, 45, 2945–2953.CrossRefGoogle Scholar

Lucey, P.G., Taylor, G.J., & Malaret, E. (1995) Abundance and distribution of iron on the Moon. Science, 268, 1150–1153.Google Scholar

Lucey, P.G., Blewett, D.T., & Hawke, B.R. (1998) Mapping the FeO and TiO₂ content of the lunar surface with multispectral imaging. Journal of Geophysical Research, 103, 3679–3699.CrossRefGoogle Scholar

Lucey, P.G., Blewett, D.T., Taylor, G.J., & Hawke, B.R. (2000) Imaging of lunar surface maturity. Journal of Geophysical Research, 105, 20377–20386.Google Scholar

Maxwell, R.E., Izenberg, N.R., & Holsclaw, G.M. (2016) Implications for iron and carbon in Mercury surface materials from ultraviolet reflectance. 47th Lunar Planet. Sci. Conf., Abstract #1606.Google Scholar

McClintock, W.E. & Lankton, M.R. (2007) The Mercury Atmospheric and Surface Composition Spectrometer for the MESSENGER mission. Space Science Reviews, 131, 481–522.Google Scholar

McClintock, W.E., Izenberg, N.R., Holsclaw, G.M., et al. (2008) Spectroscopic observations of Mercury’s surface reflectance during MESSENGER’s first Mercury flyby. Science, 321, 62–65.CrossRefGoogle ScholarPubMed

McCord, T.B. & Adams, J.B. (1972a) Mercury: Surface composition from the reflection spectrum. Science, 178, 745–747.Google Scholar

McCord, T.B. & Adams, J.B. (1972b) Mercury: Interpretation of optical observations. Icarus, 17, 585–588.Google Scholar

McCord, T.B. & Clark, R.N. (1979) The Mercury soil: Presence of Fe²⁺. Journal of Geophysical Research, 84, 7664–7668.Google Scholar

Murchie, S.L., Watters, T.R., Robinson, M.S., et al. (2008) Geology of the Caloris basin, Mercury: A view from MESSENGER. Science, 321, 73–77.Google Scholar

Murchie, S.L., Klima, R.L., Denevi, B.W., et al. (2015) Orbital multispectral mapping of Mercury with the MESSENGER Mercury Dual Imaging System: Evidence for the origins of plains units and low-reflectance material. Icarus, 254, 287–305.Google Scholar

Murchie, S.L, Klima, R.L., Domingue, D.L., Izenberg, N.R., Blewett, D.T., & Helbert, J. (2019) Spectral reflectance constraints on the composition and evolution of Mercury’s surface. In: Mercury: The view after MESSENGER (Solomon, S.C., Nittler, L.R., & Anderson, B.J., eds.). Cambridge University Press, Cambridge.Google Scholar

Murray, B.C., Belton, M.J.S., Danielson, G.E., et al. (1974) Venus: Atmosphere motion and structure from Mariner 10 pictures. Science, 183, 1307–1315.Google Scholar

Nittler, L.R., Starr, R.D., Weider, S.Z., et al. (2011) The major-element composition of Mercury’s surface from MESSENGER X-ray spectrometry. Science, 333, 1847–1850.CrossRefGoogle ScholarPubMed

Peplowski, P.N., Klima, R.L., Lawrence, D.J., et al. (2016) Remote sensing evidence for an ancient carbon-bearing crust on Mercury. Nature Geoscience, 9, 273–276.CrossRefGoogle Scholar

Pieters, C.M. (1993) Compositional diversity and stratigraphy of the lunar crust derived from reflectance spectroscopy. In: Remote geochemical analysis: Elemental and mineralogic composition (Pieters, C.M. & Englert, P.A.J., eds.). Cambridge University Press, Cambridge, 309–340.Google Scholar

Rava, B. & Hapke, B. (1987) An analysis of the Mariner 10 color ratio map of Mercury. Icarus, 71, 397–429.Google Scholar

Rivera-Valentin, E.G. & Barr, A.C. (2014) Impact-induced compositional variations on Mercury. Earth and Planetary Science Letters, 391, 234–242.CrossRefGoogle Scholar

Robinson, M.S. & Lucey, P.G. (1997) Recalibrated Mariner 10 color mosaics: Implications for mercurian volcanism. Science, 275, 197–200.Google Scholar

Robinson, M.S. & Taylor, G.J. (2001) Ferrous oxide in Mercury’s crust and mantle. Meteoritics and Planetary Science, 36, 841–847.Google Scholar

Robinson, M.S., Murchie, S.L., Blewett, D.T., et al. (2008) Reflectance and color variations on Mercury: Regolith processes and compositional heterogeneity. Science, 321, 66–69.Google Scholar

Solomon, S.C., McNutt, R.L. Jr., Gold, R.E., et al. (2001) The MESSENGER mission to Mercury: Scientific objectives and implementation. Planetary and Space Science, 49, 1445–1465.Google Scholar

Sprague, A.L., Kozlowski, R.W.H., Witteborn, F.C., Cruikshank, D.P., & Wooden, D.H. (1994) Mercury: Evidence for anorthosite and basalt from mid-infrared (7.3–13.5 micrometers) spectroscopy. Icarus, 109, 156–167.Google Scholar

Sprague, A.L., Hunten, D.M., & Lodders, K. (1995) Sulfur at Mercury, elemental at the poles and sulfides in the regolith. Icarus, 118, 211–215.Google Scholar

Sprague, A.L., Emery, J.P., Donaldson, K.L., Russell, R.W., Lynch, D.K., & Mazuk, A.L. (2002) Mercury: Mid-infrared (3–13.5 µm) observations show heterogeneous composition, presence of intermediate and basic soil types, and pyroxene. Meteoritics and Planetary Science, 37, 1255–1268.Google Scholar

Thomas, R.J., Rothery, D.A., Conway, S.J., & Anand, M. (2014a) Hollows on Mercury: Materials and mechanisms involved in their formation. Icarus, 229, 221–235.Google Scholar

Thomas, R.J., Rothery, D.A., Conway, S.J., & Anand, M. (2014b) Mechanisms of explosive volcanism on Mercury: Implications from its global distribution and morphology. Journal of Geophysical Research, 119, 2239–2254.Google Scholar

Trang, D., Lucey, P.G., & Izenberg, N.R. (2016) Mapping of submicroscopic carbon and iron on Mercury with radiative transfer modeling of MESSENGER VIRS reflectance spectra. 47th Lunar Planet. Sci. Conf., Abstract #1396.Google Scholar

Trask, N.J. & Guest, J.E. (1975) Preliminary geologic terrain map of Mercury. Journal of Geophysical Research, 80, 2461–2477.Google Scholar

Vander Kaaden, K.E., & McCubbin, F.M. (2015) Exotic crust formation on Mercury: Consequences of a shallow, FeO-poor mantle. Journal of Geophysical Research, 120, 195–209.Google Scholar

Vilas, F. & McCord, T.B. (1976) Mercury: Spectral reflectance measurements (0.33–1.06 μm) 1974/75. Icarus, 28, 593–599.Google Scholar

Vilas, F., Leake, M.A., & Mendell, W.W. (1984) The dependence of reflectance spectra of Mercury on surface terrain. Icarus, 59, 60–68.Google Scholar

Vilas, F., Domingue, D.L., Helbert, J., et al. (2016) Mineralogical indicators of Mercury’s hollows composition in MESSENGER color observations. Geophysical Research Letters, 43, 1450–1456, DOI:10.1002/2015GL067515.Google Scholar

Wänke, H. (1981) Constitution of terrestrial planets. Philosophical Transactions of the Royal Society of London A, 303, 287–302.Google Scholar

Wänke, H. & Dreibus, G. (1994) Water abundance and accretion history of terrestrial planets. Conference on Deep Earth and Planetary Volatiles, Lunar and Planetary Institute, Houston, TX, 46.Google Scholar

Warell, J. & Blewett, D.T. (2004) Properties of the hermean regolith: V. New optical reflectance spectra, comparison with lunar anorthosites, and mineralogical modeling. Icarus, 168, 257–276.Google Scholar

Warell, J., Sprague, A.L., Emery, J.P., Kozlowski, R.W.H., & Long, A. (2006) The 0.7–5.3 μm spectra of Mercury and the Moon: Evidence for high-Ca pyroxene on Mercury. Icarus, 180, 281–291.Google Scholar

Weider, S.Z., Nittler, L.R., Starr, R.D., et al. (2012) Chemical heterogeneity on Mercury’s surface revealed by the MESSENGER X-Ray Spectrometer. Journal of Geophysical Research, 117, E00L05, DOI:10.1029/2012JE004153.CrossRefGoogle Scholar

Weider, S.Z., Nittler, L.R., Starr, R.D., McCoy, T.J., & Solomon, S.C. (2014) Variations in the abundance of iron on Mercury’s surface from MESSENGER X-Ray Spectrometer observations. Icarus, 235, 170–186.Google Scholar

Weider, S.Z., Nittler, L.R., Starr, R.D., et al. (2015) Evidence for geochemical terranes on Mercury: Global mapping of major elements with MESSENGER’s X-Ray Spectrometer. Earth and Planetary Science Letters, 416, 109–120.Google Scholar

Weider, S.Z., Nittler, L.R., Murchie, S.L., et al. (2016) Evidence from MESSENGER for sulfur- and carbon-driven explosive volcanism on Mercury. Geophysical Research Letters, 43, 3653–3661, DOI:10.1002/2016GL068325.Google Scholar

Whitten, J.L., Head, J.W., Denevi, B.W., & Solomon, S.C. (2014) Intercrater plains on Mercury: Insights into unit definition, characterization, and origin from MESSENGER datasets. Icarus, 241, 97–113.Google Scholar

Zolotov, M. (2011) On the chemistry of mantle and magmatic volatiles on Mercury. Icarus, 212, 24–41.Google Scholar

Zolotov, M., Sprague, A.L., Hauck, S.A. II, Nittler, L.R., Solomon, S.C., & Weider, S.Z. (2013) The redox state, FeO content, and origin of sulfur-rich magmas on Mercury. Journal of Geophysical Research, 118, 138–146.Google Scholar

Adams, J. & McCord, T. (1970) Remote sensing of lunar surface mineralogy: Implications from visible and near-infrared reflectivity of Apollo 11 samples. Geochimica et Cosmochimica Acta Supplement, 1, 1937.Google Scholar

Adams, J.B. (1974) Visible and near-infrared diffuse reflectance spectra of pyroxenes as applied to remote sensing of solid objects in the Solar System. Journal of Geophysical Research, 79, 4829–4836.Google Scholar

Adams, J.B. & Jones, R.L. (1970) Spectral reflectivity of lunar samples. Science, 167, 737–739.Google Scholar

Adams, J.B., Pieters, C., & McCord, T.B. (1974) Orange glass: Evidence for regional deposits of pyroclastic origin on the moon. Proceedings of the 5th Lunar Planet. Sci. Conf., 171–186.Google Scholar

Bandfield, J.L., Poston, M.J., Klima, R.L., & Edwards, C.S. (2018) Widespread distribution of OH/H₂O on the lunar surface inferred from spectral data. Nature Geoscience, 11(3), 173–177.Google Scholar

Bell, P., Mao, H., & Weeks, R. (1976) Optical spectra and electron paramagnetic resonance of lunar and synthetic glasses: A study of the effects of controlled atmosphere, composition, and temperature. Proceedings of the Lunar Planet. Sci. Conf., 2543–2559.Google Scholar

Bell, P.M. & Mao, H.K. (1973) Optical and chemical analysis of iron in Luna 20 plagioclase. Geochimica et Cosmochimica Acta, 37, 755–759.Google Scholar

Bender, H.A., Mouroulis, P., Smith, C.D., et al. (2015) Snow and water imaging spectrometer (SWIS): Optomechanical and system design for a CubeSat-compatible instrument. In: Imaging Spectrometry XX (Pagano, T.S. & Silny, J.F, eds.). SPIE Proceedings, 9611.Google Scholar

Besse, S., Sunshine, J., & Gaddis, L. (2014) Volcanic glass signatures in spectroscopic survey of newly proposed lunar pyroclastic deposits. Journal of Geophysical Research, 119, 355–372.Google Scholar

Bhattacharya, S., Saran, S., Dagar, A., et al. (2013) Endogenic water on the Moon associated with non-mare silicic volcanism: Implications for hydrated lunar interior. Current Science, 105, 685–691.Google Scholar

Blewett, D.T., Coman, E.I., Hawke, B.R., Gillis-Davis, J.J., Purucker, M.E., & Hughes, C.G. (2011) Lunar swirls: Examining crustal magnetic anomalies and space weathering trends. Journal of Geophysical Research, 116, E02002, DOI:10.1029/2010JE003656.Google Scholar

Boardman, J.W., Pieters, C.M., Green, R.O., et al. (2011) Measuring moonlight: An overview of the spatial properties, lunar coverage, selenolocation, and related Level 1B products of the Moon Mineralogy Mapper. Journal of Geophysical Research, 116, E00G14, DOI:10.1029/2010JE003730.Google Scholar

Boyd, A.K., Robinson, M.S., & Sato, H. (2012) Lunar Reconnaissance Orbiter wide angle camera photometry: An empirical solution. 43rd Lunar Planet. Sci. Conf., Abstract # 2795.Google Scholar

Burns, R.G. (1993) Mineralogical applications of crystal field theory. Cambridge University Press, Cambridge.Google Scholar

Cahill, J.T., Lucey, P.G., Gillis, J.J., & Steutel, D. (2004) Verification of quality and compatibility for the newly calibrated Clementine NIR data set. 35th Lunar Planet. Sci., Abstract #1469.Google Scholar

Charette, M.P., McCord, T.B., Pieters, C., & Adams, J.B. (1974) Application of remote spectral reflectance measurements to lunar geology classification and determination of titanium content of lunar soils. Journal of Geophysical Research, 79, 1605–1613.Google Scholar

Cheek, L., Pieters, C.M., Parman, S., Dyar, M.D., Speicher, E.A., & Cooper, R.F. (2011a) Spectral characteristics of plagioclase with variable iron content: Applications to remote sensing of the lunar crust. 42nd Lunar Planet. Sci. Conf., Abstract #1617.Google Scholar

Cheek, L.C. & Pieters, C.M. (2014) Reflectance spectroscopy of plagioclase-dominated mineral mixtures: Implications for characterizing lunar anorthosites remotely. American Mineralogist, 99, 1871–1892.Google Scholar

Cheek, L.C., Pieters, C.M., Boardman, J.W., et al. (2011) Goldschmidt crater and the Moon’s north polar region: Results from the Moon Mineralogy Mapper (M³). Journal of Geophysical Research, 116, E00G02, DOI:10.1029/2010je003702.Google Scholar

Cheek, L.C., Donaldson, H.K.L., Pieters, C.M., Head, J.W., & Whitten, J.L. (2013) The distribution and purity of anorthosite across the Orientale Basin: New perspectives from Moon Mineralogy Mapper data. Journal of Geophysical Research, 118, 1805–1820.Google Scholar

Clark, R.N. (1979) Planetary reflectance measurements in the region of planetary thermal emission. Icarus, 40, 94–103.Google Scholar

Clark, R.N. (2009) Detection of adsorbed water and hydroxyl on the Moon. Science, 326, 562–564.Google Scholar

Clark, R.N., Pieters, C.M., Green, R.O., Boardman, J.W., & Petro, N.E. (2011) Thermal removal from near-infrared imaging spectroscopy data of the Moon. Journal of Geophysical Research, 116, E00G16, DOI:10.1029/2010JE003751.Google Scholar

Cloutis, E.A. & Gaffey, M.J. (1991) Spectral-compositional variations in the constituent minerals of mafic and ultramafic assemblages and remote sensing implications. Earth, Moon, and Planets, 53, 11–53.Google Scholar

Cloutis, E.A., Sunshine, J.M., & Morris, R.V. (2004) Spectral reflectance–compositional properties of spinels and chromites: Implications for planetary remote sensing and geothermometry. Meteoritics and Planetary Science, 39, 545–565.Google Scholar

Conel, J.E. & Nash, D.B. (1970) Spectral reflectance and albedo of Apollo 11 lunar samples: Effects of irradiation and vitrification and comparison with telescopic observations. Apollo 11 Lunar Sci. Conf., 2013–2023.Google Scholar

Crites, S.T., Lucey, P.G., & Taylor, G.J. (2015) The mafic component of the lunar crust: Constraints on the crustal abundance of mantle and intrusive rock, and the mineralogy of lunar anorthosites. American Mineralogist, 100, 1708–1716.Google Scholar

Denevi, B.W., Robinson, M.S., Boyd, A.K., Sato, H., Hapke, B.W., & Hawke, B.R. (2014) Characterization of space weathering from Lunar Reconnaissance Orbiter Camera ultraviolet observations of the Moon. Journal of Geophysical Research, 119, 976–997.Google Scholar

Dhingra, D., Pieters, C.M., & Head, J.W. (2015) Multiple origins for olivine at Copernicus crater. Earth and Planetary Science Letters, 420, 95–101.Google Scholar

Donaldson Hanna, K.L., Cheek, L.C., Pieters, C.M., et al. (2014) Global assessment of pure crystalline plagioclase across the Moon and implications for the evolution of the primary crust. Journal of Geophysical Research, 119, 1516–1545.Google Scholar

Dyar, M.D., Hibbitts, C.A., & Orlando, T.M. (2010) Mechanisms for incorporation of hydrogen in and on terrestrial planetary surfaces. Icarus, 208, 425–437.Google Scholar

Eliason, E., Isbell, C., Lee, E., et al. (1999) Mission to the Moon: The Clementine UVVIS Global Mosaic. PDS CL_4001–4078. www.lpi.usra.edu/lunar/tools/clementine/instructions/UVVIS_DIM_Info.htmlGoogle Scholar

Eliason, E.M., Lee, E.M., Becker, T.L., et al. (2003) A near-infrared (NIR) global multispectral map of the Moon from Clementine. 34th Lunar Planet. Sci. Conf., Abstract #2093.Google Scholar

Feldman, W.C., Maurice, S., Binder, A.B., Barraclough, B.L., Elphic, R.C., & Lawrence, D.J. (1998) Fluxes of fast and epithermal neutrons from lunar Prospector: Evidence for water ice at the lunar poles. Science, 281, 1496–1500.Google Scholar

Gaddis, L.R., Staid, M.I., Tyburczy, J.A., Hawke, B.R., & Petro, N.E. (2003) Compositional analyses of lunar pyroclastic deposits. Icarus, 161, 262–280.Google Scholar

Giguere, T.A., Taylor, G.J., Hawke, B.R., & Lucey, P.G. (2000) The titanium contents of lunar mare basalts. Meteoritics and Planetary Science, 35, 193–200.Google Scholar

Green, R. (2016) 30 years of thermally controlled imaging spectrometers for Earth and planetary science. 46th International Conference on Environmental Systems.Google Scholar

Green, R., Pieters, C.M., Mouroulis, P., et al. (2011) The Moon Mineralogy Mapper (M³) imaging spectrometer for lunar science: Instrument description, calibration, on-orbit measurements, science data calibration and on-orbit validation. Journal of Geophysical Research, 116, E00G19, DOI:10.1029/2011JE003797.Google Scholar

Hapke, B. (2001) Space weathering from Mercury to the asteroid belt. Journal of Geophysical Research, 106, 10039–10073.Google Scholar

Hawke, B.R., Peterson, C.A., Blewett, D.T., et al. (2003) Distribution and modes of occurrence of lunar anorthosite. Journal of Geophysical Research, 108, 5050, DOI:10.1029/2002JE001890.Google Scholar

Hazen, R.M., Bell, P.M., & Mao, H.K. (1978) Effects of compositional variation on absorption spectra of lunar pyroxenes. Proceedings of the 9th Lunar Planet. Sci. Conf., 2919–2934.Google Scholar

Heiken, G., Vaniman, D., & French, B.M. (1991) Lunar sourcebook: A user’s guide to the Moon. Cambridge University Press, New York.Google Scholar

Hiroi, T., Pieters, C., & Morris, R. (1997) New considerations for estimating lunar soil maturity from VIS-NIR reflectance spectroscopy. 28th Lunar Planet. Sci. Conf., Abstract #1152.Google Scholar

Hook, S.J., Johnson, W.R., & Abrams, M.J. (2013) NASA’s Hyperspectral Thermal Emission Spectrometer (HyTES). In: Thermal infrared remote sensing: Sensors, methods, applications (Kuenzer, C. & Dech, S., eds.). Springer, Dordrecht, 93–115.Google Scholar

Isaacson, P.J. & Pieters, C.M. (2009) Northern Imbrium noritic anomaly. Journal of Geophysical Research, 114, E09007, DOI:10.1029/2008JE003293.Google Scholar

Isaacson, P.J., Sarbadhikari, A.B., Pieters, C.M., et al. (2011a) The lunar rock and mineral characterization consortium: Deconstruction and integrated mineralogical, petrologic, and spectroscopic analyses of mare basalts. Meteoritics and Planetary Science, 46, 228–251.Google Scholar

Isaacson, P.J., Pieters, C.M., Besse, S., et al. (2011b) Remote compositional analysis of lunar olivine rich lithologies with Moon Mineralogy Mapper (M³) spectra. Journal of Geophysical Research, 116, E00G11, DOI:10.1029/2010JE003731.Google Scholar

Johnson, J.R. & Hörz, F. (2003) Visible/near-infrared spectra of experimentally shocked plagioclase feldspars. Journal of Geophysical Research, 108, 5120, DOI:10.1029/2003JE002127.Google Scholar

Jolliff, B.I., Wieczorek, M.A., Shearer, C.K., & Neal, C.R. (2006) New views of the Moon. Reviews in Mineralogy and Geochemistry, 60. Geochemical Society.Google Scholar

Jolliff, B.L., Wiseman, S.A., Lawrence, S.J., et al. (2011) Non-mare silicic volcanism on the lunar farside at Compton–Belkovich. Nature Geoscience, 4, 566–571.Google Scholar

Keller, L. & Zhang, S. (2015) Rates of space weathering in lunar soils. Space Weathering of Airless Bodies: An Integration of Remote Sensing Data, Laboratory Experiments and Sample Analysis Workshop, Abstract #2056.Google Scholar

Keller, L., Berger, E., Christoffersen, R., & Zhang, S. (2016) Direct determination of the space weathering rates in lunar soils and Itokawa regolith from sample analyses. 47th Lunar Planet. Sci. Conf., Abstract #2525.Google Scholar

Keller, L.P. & McKay, D.S. (1993) Discovery of vapor deposits in the lunar regolith. Science, 261, 1305–1307.Google Scholar

Keller, L.P. & McKay, D.S. (1997) The nature and origin of rims on lunar soil grains. Geochimica et Cosmochimica Acta, 61, 2331–2341.Google Scholar

Klima, R., Cahill, J., Hagerty, J., & Lawrence, D. (2013) Remote detection of magmatic water in Bullialdus crater on the Moon. Nature Geoscience, 6, 737–741.Google Scholar

Klima, R., Buczkowski, D., Ernst, C., & Greenhagen, B. (2017) Geological and spectral analysis of low-calcium pyroxenes around the Imbrium Basin on the Moon. 48th Lunar Planet. Sci. Conf., Abstract #2502.Google Scholar

Klima, R.L. & Petro, N.E. (2017) Remotely distinguishing and mapping endogenic water on the Moon. Philosophical Transactions of the Royal Society A, 375, 20150391.Google Scholar

Klima, R.L., Pieters, C.M., & Dyar, M.D. (2007) Spectroscopy of synthetic Mg-Fe pyroxenes I: Spin-allowed and spin-forbidden crystal field bands in the visible and near-infrared. Meteoritics and Planetary Science, 42, 235–253.Google Scholar

Klima, R.L., Pieters, C.M., & Dyar, M.D. (2008) Characterization of the 1.2 micrometer M1 pyroxene band: Extracting cooling history from near-IR spectra of pyroxenes and pyroxene-dominated rocks. Meteoritics and Planetary Science, 43, 1591–1604.Google Scholar

Klima, R.L., Dyar, M.D., & Pieters, C.M. (2011a) Near-infrared spectra of clinopyroxenes: Effects of calcium content and crystal structure. Meteoritics and Planetary Science, 46, 379–395.Google Scholar

Klima, R.L., Pieters, C.M., Boardman, J.W., et al. (2011b) New insights into lunar petrology: Distribution and composition of prominent low Ca pyroxene exposures as observed by the Moon Mineralogy Mapper (M³). Journal of Geophysical Research, 116, DOI:10.1029/2010JE003719.Google Scholar

Kramer, G.Y., Besse, S., Dhingra, D., et al. (2011a) M³ spectral analysis of lunar swirls and the link between optical maturation and surface hydroxyl formation at magnetic anomalies. Journal of Geophysical Research, 116, E00G18, DOI:10.1029/2010JE003729.Google Scholar

Kramer, G.Y., Besse, S., Nettles, J., et al. (2011b) Newer views of the Moon: Comparing spectra from Clementine and the Moon Mineralogy Mapper. Journal of Geophysical Research, 116, E00G04, DOI:10.1029/2010JE003728.Google Scholar

Kramer, G.Y., Kring, D.A., Nahm, A.L., & Pieters, C.M. (2013) Spectral and photogeologic mapping of Schrödinger Basin and implications for post-South Pole-Aitken impact deep subsurface stratigraphy. Icarus, 223, 131–148.Google Scholar

Li, S. & Milliken, R.E. (2016a) An empirical thermal correction model for Moon Mineralogy Mapper data constrained by laboratory spectra and Diviner temperatures. Journal of Geophysical Research, 121, 2081–2107.Google Scholar

Li, S. & Milliken, R.E. (2016b) Heterogeneous water content in the lunar interior: Insights from orbital detection of water in pyroclastic deposits and silicic domes. 47th Lunar Planet. Sci. Conf., Abstract #1568.Google Scholar

Li, S. & Milliken, R.E. (2017) Water on the surface of the Moon as seen by the Moon Mineralogy Mapper: Distribution, abundance, and origins. Science Advances, 3, e1701471.Google Scholar

LSCC data. Spectra: www.planetary.brown.edu/relabdocs/LSCCsoil.html; Composition: pgi.utk.edu/lunar-soil-characterization-consortium-lscc-data/Google Scholar

Lucey, P.G. (2004) Planets-L08701. Mineral maps of the Moon. Geophysical Research Letters, 31, L08701, DOI:10.1029/2003GL019406.Google Scholar

Lucey, P.G., Blewett, D.T., & Hawke, B.R. (1998) Mapping the FeO and TiO₂ content of the lunar surface with multispectral imagery. Journal of Geophysical Research, 103, 3679–3699.Google Scholar

Lucey, P.G., Blewett, D.T., Eliason, E.M., et al. (2000) Optimized calibration constants for the Clementine NIR camera. 31st Lunar Planet. Sci. Conf., Abstract #1273.Google Scholar

Lucey, P.G., Norman, J.A., Crites, S.T., et al. (2014) A large spectral survey of small lunar craters: Implications for the composition of the lunar mantle. American Mineralogist, 99, 2251–2257.Google Scholar

Lundeen, S., McLaughlin, S., & Alanis, R. (2011) Moon Mineralogy Mapper Data Product software interface specification. PDS document Version 9.10. Jet Propulsion Laboratory, JPL D-39032, Pasadena, CA.Google Scholar

McCord, T.B. & Johnson, T.V. (1970) Lunar spectral reflectivity (0.30 to 2.50 microns) and implications for remote mineralogical analysis. Science, 169, 855–858.Google Scholar

McCord, T.B., Clark, R.N., Hawke, B.R., et al. (1981) Moon: Near-infrared spectral reflectance, a first good look. Journal of Geophysical Research, 86, 10883–10892.Google Scholar

McCord, T.B., Taylor, L.A., Combe, J.P., et al. (2011) Sources and physical processes responsible for OH/H₂O in the lunar soil as revealed by the Moon Mineralogy Mapper (M³). Journal of Geophysical Research, 116, E00G05, DOI:10.1029/2010JE003711.Google Scholar

McEwen, A.S. & Robinson, M. (1997) Mapping of the Moon by Clementine. Advances in Space Research, 19(10), 1523–1533.Google Scholar

McEwen, A.S., Eliason, E., Lucey, P., et al. (1998) Summary of radiometric calibration and photometric normalization steps for the Clementine UVVIS images. 29th Lunar Planet. Sci. Conf., Abstract 1466–1467.Google Scholar

Milliken, R.E. & Li, S. (2017) Remote detection of widespread indigenous water in lunar pyroclastic deposits. Nature Geoscience, 10, 561–565.Google Scholar

Moriarty III, D.P. & Pieters, C.M. (2016a) South Pole–Aitken Basin as a probe to the lunar interior. 47th Lunar Planet. Sci. Conf., Abstract #1763.Google Scholar

Moriarty III, D.P. & Pieters, C.M. (2016b) Complexities in pyroxene compositions derived from absorption band centers: Examples from Apollo samples, HED meteorites, synthetic pure pyroxenes, and remote sensing data. Meteoritics and Planetary Science, 51, 207–234.Google Scholar

Moriarty III, D.P. & Pieters, C.M. (2018) The character of South Pole-Aitken Basin: Patterns of surface and subsurface composition. Journal of Geophysical Research, 123, 729–747.Google Scholar

Mouroulis, P., Green, R.O., & Chrien, T.G. (2000) Design of pushbroom imaging spectrometers for optimum recovery of spectroscopic and spatial information. Applied Optics, 39, 2210–2220.Google Scholar

Nakamura, R., Yamamoto, S., Matsunaga, T., et al. (2012) Compositional evidence for an impact origin of the Moon’s Procellarum basin. Nature Geoscience, 5(11),775–778, DOI:10.1038/ngeo1614.Google Scholar

National Research Council, Space Studies Board. (2007) Scientific context for exploration of the Moon. National Academies Press, Washington, DC.Google Scholar

Noble, S.K., Pieters, C.M., Hiroi, T., & Taylor, L.A. (2006) Using the modified Gaussian model to extract quantitative data from lunar soils. Journal of Geophysical Research, 111, DOI:10.1029/2006JE002721.Google Scholar

Noble, S.K., Pieters, C.M., & Keller, L.P. (2007) An experimental approach to understanding the optical effects of space weathering. Icarus, 192, 629–642.Google Scholar

Nozette, S., Rustan, P., Pleasance, L.P., et al. (1994) The Clementine Mission to the Moon: Scientific overview. Science, 266, 1835–1839.Google Scholar

Ohtake, M., Matsunaga, T., Haruyama, J., et al. (2009) The global distribution of pure anorthosite on the Moon. Nature, 461, 236–240.Google Scholar

Ohtake, M., Matsunaga, T., Yokota, Y., et al. (2010) Deriving the absolute reflectance of lunar surface using SELENE (Kaguya) multiband imager data. Space Science Reviews, 154, 57–77.Google Scholar

Ohtake, M., Pieters, C., Isaacson, P., et al. (2013) One Moon, many measurements 3: Spectral reflectance. Icarus, 226, 364–374.Google Scholar

Petro, N.E., Isaacson, P.J., Pieters, C.M., Jolliff, B.L., Carter, L.M., & Klima, R.L. (2013) Presence of OH/H₂O associated with the lunar Compton-Belkovich volcanic complex identified by the Moon Mineralogy Mapper (M³). 44th Lunar Planet. Sci. Conf., 2688.Google Scholar

Pieters, C.M. (1978) Mare basalt types on the front side of the moon: A summary of spectral reflectance data. Proceedings of the 9th Lunar Sci. Conf. (Suppl. 10, Geochimica et Cosmochimica Acta), 2825–2849.Google Scholar

Pieters, C.M. (1982) Copernicus crater central peak: Lunar mountain of unique composition. Science, 215, 59–61.Google Scholar

Pieters, C.M. (1993) Compositional diversity and stratigraphy of the Lunar crust derived from reflectance spectroscopy. In: Remote geochemical analysis: Elemental and mineralogical composition (Pieters, C. & Englert, P., eds.). Cambridge University Press, Cambridge, 309–339.Google Scholar

Pieters, C.M. (1996) Plagioclase and maskelynite diagnostic features. 27th Lunar Planet. Science Conf., Abstract #1031.Google Scholar

Pieters, C.M. (2017) Origin and importance of “featureless” plagioclase on the Moon. 5th Eur. Lunar Symp., Munster, Germany.Google Scholar

Pieters, C.M. & Garrick-Bethell, I. (2015) Hydration variations at lunar swirls. 46th Lunar Planet. Sci. Conf., Abstract #2120.Google Scholar

Pieters, C.M. & Noble, S.K. (2016) Space weathering on airless bodies. Journal of Geophysical Research, 121, 1865–1884.Google Scholar

Pieters, C.M. & Taylor, L.A. (2003) Systematic global mixing and melting in lunar soil evolution. Geophysical Research Letters, 30, 2048, DOI:10.1029/2003GL018212.Google Scholar

Pieters, C.M., Head, J.W., Adams, J.B., McCord, T.B., Zisk, S.H., & Whitford Stark, J.L. (1980) Late high titanium basalts of the western maria: Geology of the Flamsteed region of Oceanus Procellarum. Journal of Geophysical Research, 85, 3913–3938.Google Scholar

Pieters, C.M., Taylor, L.A., Noble, S.K., et al. (2000) Space weathering on airless bodies: Resolving a mystery with lunar samples. Meteoritics and Planetary Science, 35, 1101–1107.Google Scholar

Pieters, C.M., Head III, J.W., Gaddis, L.R., Jolliff, B.L., & Duke, M. (2001) Rock types of South Pole-Aitken Basin and extent of basaltic volcanism. Journal of Geophysical Research, 106, 28,001–28,022.Google Scholar

Pieters, C.M., Boardman, J., Buratti, B., et al. (2009a) Mineralogy of the lunar crust in spatial context: First results from the Moon Mineralogy Mapper (M³). 40th Lunar Planet. Sci. Conf., Abstract #2052.Google Scholar

Pieters, C.M., Goswami, J.N., Clark, R., et al. (2009b) Character and spatial distribution of OH/H₂O on the surface of the Moon seen by M³ on Chandrayaan-1. Science, 326, 568–572.Google Scholar

Pieters, C.M., Besse, S., & Boardman, J. (2011) Mg spinel lithology: A new rock type on the lunar farside. Journal of Geophysical Research, 116, E00G08, DOI:10.1029/2010JE003727.Google Scholar

Pieters, C.M., Boardman, J.W., Ohtake, M., et al. (2013) One Moon, many measurements 1: Radiance values. Icarus, 226, 951–963.Google Scholar

Pieters, C.M., Hanna, K.D., Cheek, L., et al. (2014) The distribution of Mg-spinel across the Moon and constraints on crustal origin. American Mineralogist, 99, 1893–1910.Google Scholar

Prissel, T., Parman, S., Jackson, C., et al. (2014) Pink Moon: The petrogenesis of pink spinel anorthosites and implications concerning Mg-suite magmatism. Earth and Planetary Science Letters, 403, 144–156.Google Scholar

Robinson, M., Brylow, S., Tschimmel, M., et al. (2010) Lunar Reconnaissance Orbiter Camera (LROC) instrument overview. Space Science Reviews, 150, 81–124.Google Scholar

Sasaki, S., Nakamura, K., Hamabe, Y., Kurahashi, E., & Hiroi, T. (2001) Production of iron nanoparticles by laser irradiation in a simulation of lunar-like space weathering. Nature, 410, 555–557.Google Scholar

Staid, M.I. & Pieters, C.M. (2001) Mineralogy of the last lunar basalts: Results from Clementine. Journal of Geophysical Research, 106, 27887–27900.Google Scholar

Staid, M.I., Pieters, C.M., Besse, S., et al. (2011) The mineralogy of late stage lunar volcanism as observed by the Moon Mineralogy Mapper on Chandrayaan 1. Journal of Geophysical Research, 116, E00G10, DOI:10.1029/2010JE003735.Google Scholar

Stöffler, D. (1972) Deformation and transformation of rock-forming minerals by natural and experimental shock processes. 1.Behavior of minerals under shock compression. Fortschritte der Mineralogie, 49, 50–113.Google Scholar

Stöffler, D. (1974) Deformation and transformation of rock-forming minerals by natural and experimental shock processes: II. Physical properties of shocked minerals. Fortschritte der Mineralogie, 51, 256–289.Google Scholar

Sun, Y.S. & Li, L.L. (2015) Characterization of lunar crust mineralogy with M³ data. 46th Lunar Planet. Sci. Conf., Abstract #2941.Google Scholar

Sunshine, J.M. & Pieters, C.M. (1993) Estimating modal abundances from the spectra of natural and laboratory pyroxene mixtures using the modified Gaussian model. Journal of Geophysical Research, 98, 9075–9087.Google Scholar

Sunshine, J.M., Farnham, T.L., Feaga, L.M., et al. (2009) Temporal and spatial variability of lunar hydration as observed by the Deep Impact spacecraft. Science, 326, 565–568.Google Scholar

Taylor, L.A., Pieters, C.M., Keller, L.P., Morris, R.V., & McKay, D.S. (2001) Lunar mare soils: Space weathering and the major effects of surface correlated nanophase Fe. Journal of Geophysical Research, 106, 27,985–27,999.Google Scholar

Taylor, L.A., Pieters, C., Patchen, A., et al. (2010) Mineralogical and chemical characterization of lunar highland soils: Insights into the space weathering of soils on airless bodies. Journal of Geophysical Research, 115, E02002, DOI:10.1029/2009JE003427.Google Scholar

Tompkins, S. & Pieters, C.M. (1999) Mineralogy of the lunar crust: Results from Clementine. Meteoritics and Planetary Science, 34, 25–41.Google Scholar

Tompkins, S. & Pieters, C.M. (2010) Spectral characteristics of lunar impact melts and inferred mineralogy. Meteoritics and Planetary Science, 45, 1152–1169.Google Scholar

Van Gorp, B., Mouroulis, P., Blaney, D.L., Green, R.O., Ehlmann, B.L., & Rodriguez, J.I. (2014) Ultra-compact imaging spectrometer for remote, in situ, and microscopic planetary mineralogy. Journal of Applied Remote Sensing, 8, 084988.Google Scholar

Vane, G. (1993) Imaging spectrometry of the Earth and other Solar System bodies. In: Remote geochemical analysis: Elemental and mineralogical composition (Pieters, C.M. & Englert, P.A.J., eds.). Cambridge University Press, Cambridge, 121–143.Google Scholar

Watson, K., Murray, B.C., & Brown, H. (1961) The behavior of volatiles on the lunar surface. Journal of Geophysical Research, 66, 3033–3045.Google Scholar

Yamamoto, S., Nakamura, R., Matsunaga, T., et al. (2010) Possible mantle origin of olivine around lunar impact basins detected by SELENE. Nature Geoscience, 3, 533–536.Google Scholar

Yamamoto, S., Matsunaga, T., Ogawa, Y., et al. (2011) Preflight and in-flight calibration of the spectral profiler on board SELENE (Kaguya). IEEE Transactions on Geoscience and Remote Sensing, 49, 4660–4676.Google Scholar

Yamamoto, S., Matsunaga, T., Ogawa, Y., et al. (2014) Calibration of NIR 2 of spectral profiler onboard Kaguya/SELENE. IEEE Transactions on Geoscience and Remote Sensing, 52, 6882–6898.Google Scholar

Yamamoto, S., Nakamura, R., Matsunaga, T., et al. (2015) Featureless spectra on the Moon as evidence of residual lunar primordial crust. Journal of Geophysical Research, 120, 2190–2205.Google Scholar

Abe, M., Takagi, Y., Kitazato, K., et al. (2006) Near-infrared spectral results of asteroid Itokawa from the Hayabusa spacecraft. Science, 312, 1334–1338.Google Scholar

Adams, J.B. (1974) Visible and near‐infrared diffuse reflectance spectra of pyroxenes as applied to remote sensing of solid objects in the Solar System. Journal of Geophysical Research, 79, 4829–4836.Google Scholar

Barucci, M., Fornasier, S., Dotto, E., et al. (2008) Asteroids 2867 Steins and 21 Lutetia: Surface composition from far infrared observations with the Spitzer space telescope. Astronomy and Astrophysics, 477, 665–670.Google Scholar

Barucci, M., Belskaya, I., Fornasier, S., et al. (2012) Overview of Lutetia’s surface composition. Planetary and Space Science, 66, 23–30.Google Scholar

Barucci, M.A., Fulchignoni, M., Ji, J., Marchi, S., & Thomas, N. (2015) The flybys of asteroids (2867) Šteins, (21) Lutetia, and (4179) Toutatis. In: Asteroids IV (Michel, P., DeMeo, F.E., & Bottke, W.F., eds.). University of Arizona Press, Tucson, 433–450.Google Scholar

Bell, J. III, Izenberg, N., Lucey, P., et al. (2002) Near-IR reflectance spectroscopy of 433 Eros from the NIS instrument on the NEAR mission: I. Low phase angle observations. Icarus, 155, 119–144.Google Scholar

Binzel, R.P., Burbine, T.H., & Bus, S.J. (1996) Groundbased reconnaissance of asteroid 253 Mathilde: Visible wavelength spectrum and meteorite comparison. Icarus, 119, 447–449.Google Scholar

Binzel, R.P., Rivkin, A.S., Bus, S.J., Sunshine, J.M., & Burbine, T.H. (2001) MUSES‐C target asteroid (25143) 1998 SF36: A reddened ordinary chondrite. Meteoritics and Planetary Science, 36, 1167–1172.Google Scholar

Bobrovnikoff, N.T. (1929) The spectra of minor planets. Lick Observatory Bulletin, 14, 18–27.Google Scholar

Brucato, J.R., Strazzulla, G., Baratta, G., & Colangeli, L. (2004) Forsterite amorphisation by ion irradiation: Monitoring by infrared spectroscopy. Astronomy and Astrophysics, 413, 395–401.Google Scholar

Brunetto, R., Loeffler, M.J., Nesvorný, D., Sasaki, S., & Strazzulla, G. (2015) Asteroid surface alteration by space weathering processes. In: Asteroids IV (Michel, P., DeMeo, F.E., & Bottke, W.F., eds.). University of Arizona Press, Tucson, 597–616.Google Scholar

Burbine, T.H. & Binzel, R.P. (2002) Small main-belt asteroid spectroscopic survey in the near-infrared. Icarus, 159, 468–499.Google Scholar

Burbine, T.H., Buchanan, P.C., Dolkar, T., & Binzel, R.P. (2009) Pyroxene mineralogies of near‐Earth vestoids. Meteoritics and Planetary Science, 44, 1331–1341.Google Scholar

Bus, S.J. & Binzel, R.P. (2002) Phase II of the small main-belt asteroid spectroscopic survey: The observations. Icarus, 158, 106–145.Google Scholar

Carvano, J.M., Hasselmann, P.H., Lazzaro, D., & Mothé-Diniz, T. (2010) SDSS-based taxonomic classification and orbital distribution of main belt asteroids. Astronomy and Astrophysics, 510, A43.Google Scholar

Chapman, C.R., Morrison, D., & Zellner, B. (1975) Surface properties of asteroids: A synthesis of polarimetry, radiometry, and spectrophotometry. Icarus, 25, 104–130.Google Scholar

Clark, B.E., Veverka, J., Helfenstein, P., et al. (1999) NEAR photometry of Asteroid 253 Mathilde. Icarus, 140, 53–65.Google Scholar

Clark, B.E., Bus, S.J., Rivkin, A.S., et al. (2004) E‐type asteroid spectroscopy and compositional modeling. Journal of Geophysical Research, 109, DOI:10.1029/2003JE002200.Google Scholar

Clark, R.N. (2009) Detection of adsorbed water and hydroxyl on the Moon. Science, 326, 562–564.Google Scholar

Cloutis, E.A., Gaffey, M.J., Jackowski, T.L., & Reed, K.L. (1986) Calibrations of phase abundance, composition, and particle size distribution for olivine‐orthopyroxene mixtures from reflectance spectra. Journal of Geophysical Research, 91, 11641–11653.Google Scholar

Cochran, A.L. & Vilas, F. (1997) The McDonald Observatory serendipitous UV/blue spectral survey of asteroids. Icarus, 127, 121–129.Google Scholar

Cohen, M., Witteborn, F.C., Roush, T., Bregman, J., & Wooden, D. (1998) Spectral irradiance calibration in the infrared. VIII. 5–14 micron spectroscopy of the asteroids Ceres, Vesta, and Pallas. The Astronomical Journal, 115, 1671–1679.CrossRefGoogle Scholar

Combe, J.-P., McCord, T.B., Tosi, F., et al. (2016) Detection of local H₂O exposed at the surface of Ceres. Science, 353, aaf3010.Google Scholar

Delbó, M., Mueller, M., Emery, J.P., Rozitis, B., & Capria, M.T. (2015) Asteroid thermophysical modeling. In: Asteroids IV (Michel, P., DeMeo, F.E., & Bottke, W.F., eds.), University of Arizona Press, Tucson, 107–128.Google Scholar

DeMeo, F.E. & Carry, B. (2013) The taxonomic distribution of asteroids from multi-filter all-sky photometric surveys. Icarus, 226, 723–741.Google Scholar

DeMeo, F.E., Binzel, R.P., Slivan, S.M., & Bus, S.J. (2009) An extension of the Bus asteroid taxonomy into the near-infrared. Icarus, 202, 160–180.Google Scholar

DeMeo, F.E., Alexander, C.M.O., Walsh, K.J., Chapman, C.R., & Binzel, R.P. (2015) The compositional structure of the asteroid belt. In: Asteroids IV (Michel, P., DeMeo, F.E., & Bottke, W.F., eds.). University of Arizona Press, Tucson, 13–41.Google Scholar

De Sanctis, M.C., Combe, J.-P., Ammannito, E., et al. (2012) Detection of widespread hydrated materials on Vesta by the VIR imaging spectrometer on board the Dawn mission. The Astrophysical Journal Letters, 758, L36.Google Scholar

De Sanctis, M.C., Ammannito, E., Raponi, A., et al. (2015) Ammoniated phyllosilicates with a likely outer Solar System origin on (1) Ceres. Nature, 528, 241–244.Google Scholar

De Sanctis, M.C., Ammannito, E., McSween, H.Y., et al. (2017) Localized aliphatic organic material on the surface of Ceres. Science, 355, 719–722.Google Scholar

Dodson-Robinson, S.E., Willacy, K., Bodenheimer, P., Turner, N.J., & Beichman, C.A. (2009) Ice lines, planetesimal composition and solid surface density in the solar nebula. Icarus, 200, 672–693.Google Scholar

Dotto, E., Müller, T., Barucci, M., et al. (2000) ISO results on bright Main Belt asteroids: PHT-S observations. Astronomy and Astrophysics, 358, 1133–1141.Google Scholar

Dunn, T.L., McCoy, T.J., Sunshine, J., & McSween, H.Y. Jr. (2010) A coordinated spectral, mineralogical, and compositional study of ordinary chondrites. Icarus, 208, 789–797.Google Scholar

Emery, J.P. & Brown, R.H. (2003) Constraints on the surface composition of Trojan asteroids from near-infrared (0.8–4.0 μm) spectroscopy. Icarus, 164, 104–121.Google Scholar

Emery, J.P. & Brown, R.H. (2004) The surface composition of Trojan asteroids: Constraints set by scattering theory. Icarus, 170, 131–152.Google Scholar

Emery, J.P., Cruikshank, D.P., & Van Cleve, J. (2006) Thermal emission spectroscopy (5.2–38 μm) of three Trojan asteroids with the Spitzer Space Telescope: Detection of fine-grained silicates. Icarus, 182, 496–512.Google Scholar

Emery, J.P., Burr, D.M., & Cruikshank, D.P. (2011) Near-infrared spectroscopy of Trojan asteroids: Evidence for two compositional groups. The Astronomical Journal, 141, 25.Google Scholar

Filippenko, A.V. (1982) The importance of atmospheric differential refraction in spectrophotometry. Publications of the Astronomical Society of the Pacific, 94, 715–721.Google Scholar

Fornasier, S., Migliorini, A., Dotto, E., & Barucci, M. (2008) Visible and near infrared spectroscopic investigation of E-type asteroids, including 2867 Steins, a target of the Rosetta mission. Icarus, 196, 119–134.Google Scholar

Fornasier, S., Clark, B., Dotto, E., Migliorini, A., Ockert-Bell, M., & Barucci, M. (2010) Spectroscopic survey of M-type asteroids. Icarus, 210, 655–673.Google Scholar

Fujiwara, A., Kawaguchi, J., Yeomans, D., et al. (2006) The rubble-pile asteroid Itokawa as observed by Hayabusa. Science, 312, 1330–1334.Google Scholar

Gaffey, M.J., Bell, J.F., Brown, R.H., et al. (1993) Mineralogical variations within the S-type asteroid class. Icarus, 106, 573–602.Google Scholar

Gladman, B.J., Davis, D.R., Neese, C., et al. (2009) On the asteroid belt’s orbital and size distribution. Icarus, 202, 104–118.Google Scholar

Gradie, J. & Tedesco, E. (1982) Compositional structure of the asteroid belt. Science, 216, 1405–1407.Google Scholar

Grossman, L. (1972) Condensation in the primitive solar nebula. Geochimica et Cosmochimica Acta, 36, 597–619.Google Scholar

Groussin, O., Lamy, P., Fornasier, S., & Jorda, L. (2011) The properties of asteroid (2867) Steins from Spitzer Space Telescope observations and OSIRIS shape reconstruction. Astronomy and Astrophysics, 529, A73.Google Scholar

Guilbert-Lepoutre, A. (2014) Survival of water ice in Jupiter Trojans. Icarus, 231, 232–238.Google Scholar

Hamilton, V.E., Simon, A.A., Christensen, P.R., et al. (2019) Evidence for widespread hydrated minerals on asteroid (101955) Bennu. Nature Astronomy, 3, 332–340.Google Scholar

Hapke, B. (2001) Space weathering from Mercury to the asteroid belt. Journal of Geophysical Research, 106, 10,039–10,073.Google Scholar

Hapke, B. (2012) Theory of reflectance and emittance spectroscopy. Cambridge University Press, Cambridge.Google Scholar

Hardersen, P.S., Cloutis, E.A., Reddy, V., Mothé-Diniz, T., & Emery, J.P. (2011) The M‐/X‐asteroid menagerie: Results of an NIR spectral survey of 45 main‐belt asteroids. Meteoritics and Planetary Science, 46, 1910–1938.Google Scholar

Hartmann, W.K., Tholen, D.J., & Cruikshank, D.P. (1987) The relationship of active comets, “extinct” comets, and dark asteroids. Icarus, 69, 33–50.Google Scholar

Hasegawa, S., Murakawa, K., Ishiguro, M., et al. (2003) Evidence of hydrated and/or hydroxylated minerals on the surface of asteroid 4 Vesta. Geophysical Research Letters, 30, DOI:10.1029/2003GL018627.Google Scholar

Hendrix, A.R., Vilas, F., & Li, J.Y. (2016) Ceres: Sulfur deposits and graphitized carbon. Geophysical Research Letters, 43, 8920–8927.Google Scholar

Henning, T. (2010) Cosmic silicates. Annual Review of Astronomy and Astrophysics, 48, 21–46.Google Scholar

Ivezić, Ž., Axelrod, T., Brandt, W., et al. (2008) Large Synoptic Survey Telescope: From science drivers to reference design. Serbian Astronomical Journal, 176, 1–13.Google Scholar

Izenberg, N.R., Murchie, S.L., Bell, J.F. III, et al. (2003) Spectral properties and geologic processes on Eros from combined NEAR NIS and MSI data sets. Meteoritics and Planetary Science, 38, 1053–1077.Google Scholar

Jones, T.D., Lebofsky, L.A., Lewis, J.S., & Marley, M.S. (1990) The composition and origin of the C, P, and D asteroids: Water as a tracer of thermal evolution in the outer belt. Icarus, 88, 172–192.Google Scholar

Kelley, M.S., Sanchez, J.A., & Reddy, V. (2017) Characterization of spacecraft targets: Ida and Gaspra. Conference on Asteroids, Comets, Meteors, Montevideo, Uruguay, poster 2.e.67.Google Scholar

King, T.V. & Ridley, W.I. (1987) Relation of the spectroscopic reflectance of olivine to mineral chemistry and some remote sensing implications. Journal of Geophysical Research, 92, 11,457–11,469.Google Scholar

Lantz, C., Brunetto, R., Barucci, M., et al. (2017) Ion irradiation of carbonaceous chondrites: A new view of space weathering on primitive asteroids. Icarus, 285, 43–57.Google Scholar

Lawrence, S.J. & Lucey, P.G. (2007) Radiative transfer mixing models of meteoritic assemblages. Journal of Geophysical Research, 112, DOI:10.1029/2006JE002765.Google Scholar

Lazzaro, D., Angeli, C., Carvano, J., Mothé-Diniz, T., Duffard, R., & Florczak, M. (2004) S 3 OS 2: The visible spectroscopic survey of 820 asteroids. Icarus, 172, 179–220.Google Scholar

Levison, H.F., Bottke, W.F., Gounelle, M., Morbidelli, A., Nesvorný, D., & Tsiganis, K. (2009) Contamination of the asteroid belt by primordial trans-Neptunian objects. Nature, 460, 364–366.Google Scholar

Lewis, J.S. (1972) Low temperature condensation from the solar nebula. Icarus, 16, 241–252.Google Scholar

Li, J.-Y., Bodewits, D., Feaga, L.M., et al. (2011) Ultraviolet spectroscopy of asteroid (4) Vesta. Icarus, 216, 640–649.Google Scholar

Lim, L.F., McConnochie, T.H., Bell, J.F. III, & Hayward, T.L. (2005) Thermal infrared (8–13 μm) spectra of 29 asteroids: The Cornell mid-infrared asteroid spectroscopy (MIDAS) survey. Icarus, 173, 385–408.Google Scholar

Lim, L.F., Emery, J.P., & Moskovitz, N.A. (2011) Mineralogy and thermal properties of V-type Asteroid 956 Elisa: Evidence for diogenitic material from the Spitzer IRS (5–35 μm) spectrum. Icarus, 213, 510–523.Google Scholar

Loeffler, M., Dukes, C., & Baragiola, R. (2009) Irradiation of olivine by 4 keV He+: Simulation of space weathering by the solar wind. Journal of Geophysical Research, 114, DOI:10.1029/2008JE003249.Google Scholar

Lord, S.D. (1992) A new software tool for computing Earth’s atmospheric transmission of near- and far-infrared radiation. NASA TM-103957. NASA Ames Research Center, Moffett Field, CA.Google Scholar

Mainzer, A., Masiero, J., Grav, T., et al. (2011a) NEOWISE studies of asteroids with Sloan photometry: Preliminary results. The Astrophysical Journal, 745, 7.Google Scholar

Mainzer, A., Bauer, J., Grav, T., et al. (2011b) Preliminary results from NEOWISE: An enhancement to the wide-field infrared survey explorer for Solar System science. The Astrophysical Journal, 731, 53.Google Scholar

Marchis, F., Enriquez, J., Emery, J., et al. (2012) Multiple asteroid systems: Dimensions and thermal properties from Spitzer Space Telescope and ground-based observations. Icarus, 221, 1130–1161.Google Scholar

Markus, K., Arnold, G., Hiesinger, H., et al. (2013) Comparison of ground-based and VIRTIS-M/ROSETTA reflectance spectra of asteroid 2867 Steins with laboratory reflectance spectra in the VIS and IR. EGU General Assembly, Abstract #EGU2013-11287.Google Scholar

Mayne, R., Sunshine, J., McSween, H. Jr., Bus, S., & McCoy, T.J. (2011) The origin of Vesta’s crust: Insights from spectroscopy of the Vestoids. Icarus, 214, 147–160.Google Scholar

McCord, T.B., Li, J.-Y., Combe, J.-P., et al. (2012) Dark material on Vesta from the infall of carbonaceous volatile-rich material. Nature, 491, 83–86.Google Scholar

McCoy, T.J., Burbine, T., McFadden, L., et al. (2001) The composition of 433 Eros: A mineralogical—chemical synthesis. Meteoritics and Planetary Science, 36, 1661–1672.Google Scholar

McFadden, L.A., Wellnitz, D.D., Schnaubelt, M., et al. (2001) Mineralogical interpretation of reflectance spectra of Eros from NEAR near‐infrared spectrometer low phase flyby. Meteoritics and Planetary Science, 36, 1711–1726.Google Scholar

McSween, Y. Jr., Ghosh, A., Grimm, R.E., Wilson, L., & Young, E.D. (2002) Thermal evolution models of asteroids. In: Asteroids III (Bottke, W., Paolicchi, Cellino, & Binzel, R.P., eds.). University of Arizona Press, Tucson, 559–571.Google Scholar

Mignard, F., Cellino, A., Muinonen, K., et al. (2007) The Gaia mission: Expected applications to asteroid science. Earth, Moon, and Planets, 101, 97–125.Google Scholar

Milliken, R.E. & Rivkin, A.S. (2009) Brucite and carbonate assemblages from altered olivine-rich materials on Ceres. Nature Geoscience, 2, 258–261.Google Scholar

Morbidelli, A., Levison, H.F., Tsiganis, K., & Gomes, R. (2005) Chaotic capture of Jupiter’s Trojan asteroids in the early Solar System. Nature, 435, 462–465.Google Scholar

Moyano‐Cambero, C.E., Trigo‐Rodrίguez, J.M., Llorca, J., Fornasier, S., Barucci, M.A., & Rimola, A. (2016) A plausible link between the asteroid 21 Lutetia and CH carbonaceous chondrites. Meteoritics and Planetary Science, 51, 1795–1812.Google Scholar

Muinonen, K. & Pieniluoma, T. (2011) Light scattering by Gaussian random ellipsoid particles: First results with discrete-dipole approximation. Journal of Quantitative Spectroscopy and Radiative Transfer, 112, 1747–1752.Google Scholar

Nakamura, T., Noguchi, T., Tanaka, M., et al. (2011) Itokawa dust particles: A direct link between S-type asteroids and ordinary chondrites. Science, 333, 1113–1116.Google Scholar

Nesvorný, D., Vokrouhlický, D., & Morbidelli, A. (2013) Capture of Trojans by jumping Jupiter. The Astrophysical Journal, 768, 45.Google Scholar

Nittler, L.R., Starr, R.D., Lim, L., et al. (2001) X‐ray fluorescence measurements of the surface elemental composition of asteroid 433 Eros. Meteoritics and Planetary Science, 36, 1673–1695.Google Scholar

O’Brien, D.P. & Sykes, M.V. (2011) The origin and evolution of the asteroid belt—Implications for Vesta and Ceres. Space Science Reviews, 163, 41–61.Google Scholar

Pieters, C.M. & Noble, S.K. (2016) Space weathering on airless bodies. Journal of Geophysical Research, 121, 1865–1884.Google Scholar

Pieters, C.M., Goswami, J.N., Clark, R.N., et al. (2009) Character and spatial distribution of OH/H₂O on the surface of the Moon seen by M3 on Chandrayaan-1. Science, 326, 568–572.Google Scholar

Popescu, M., Licandro, J., Morate, D., et al. (2016) Near-infrared colors of minor planets recovered from Vista-VHS survey (MOVIS). Astronomy and Astrophysics, 591, A115.Google Scholar

Prinn, R.G., & Fegley, B. Jr. (1989) Solar nebula chemistry: Origins of planetary, satellite and cometary volatiles. In: Origin and evolution of planetary and satellite atmospheres (Atreya, S.K., Pollack, J.B., & Matthews, M.S., eds.). University of Arizona Press, Tucson, 78–136.Google Scholar

Reddy, V., Le Corre, L., O’Brien, D.P., et al. (2012) Delivery of dark material to Vesta via carbonaceous chondritic impacts. Icarus, 221, 544–559.Google Scholar

Reddy, V., Dunn, T., Thomas, C.A., Moskovitz, N., & Burbine, T. (2015) Mineralogy and surface composition of asteroids. In: Asteroids IV (Michel, P., DeMeo, F.E., & Bottke, W.F., eds.). University of Arizona Press, Tucson, 65–87.Google Scholar

Rivkin, A.S. & Emery, J.P. (2010) Detection of ice and organics on an asteroidal surface. Nature, 464, 1322–1323.Google Scholar

Rivkin, A.S., Clark, B.E., Britt, D.T., & Lebofsky, L.A. (1997) Infrared spectrophotometry of the NEAR flyby target 253 Mathilde. Icarus, 127, 255–257.Google Scholar

Rivkin, A.S., Howell, E.S., Vilas, F., & Lebofsky, L.A. (2002) Hydrated minerals on asteroids: The astronomical record. Asteroids III, 1, 235–253.Google Scholar

Rivkin, A.S., Volquardsen, E.L., & Clark, B.E. (2006) The surface composition of Ceres: Discovery of carbonates and iron-rich clays. Icarus, 185, 563–567.Google Scholar

Rivkin, A.S., Clark, B.E., Ockert-Bell, M., et al. (2011) Asteroid 21 Lutetia at 3 μm: Observations with IRTF SpeX. Icarus, 216, 62–68.Google Scholar

Rivkin, A.S., Thomas, C.A., Howell, E.S., & Emery, J.P. (2015) The Ch-class asteroids: Connecting a visible taxonomic class to a 3 μm band shape. The Astronomical Journal, 150, 198.Google Scholar

Rivkin, A.S., Howell, E.S., Emery, J.P., & Sunshine, J. (2018) Evidence for OH or H₂O on the surface of 433 Eros and 1036 Ganymed. Icarus, 304, 74–82.Google Scholar

Russell, C.T., Raymond, C.A., Coradini, A., et al. (2012) Dawn at Vesta: Testing the protoplanetary paradigm. Science, 336, 684–686.Google Scholar

Sanchez, J.A., Reddy, V., Nathues, A., Cloutis, E.A., Mann, P., & Hiesinger, H. (2012) Phase reddening on near-Earth asteroids: Implications for mineralogical analysis, space weathering and taxonomic classification. Icarus, 220, 36–50.Google Scholar

Schorghofer, N. (2016) Predictions of depth-to-ice on asteroids based on an asynchronous model of temperature, impact stirring, and ice loss. Icarus, 276, 88–95.Google Scholar

Shestopalov, D.I., Golubeva, L.F., McFadden, L.A., Fornasier, S., & Taran, M.N. (2010) Titanium-bearing pyroxenes of some E asteroids: Coexisting of igneous and hydrated rocks. Planetary and Space Science, 58, 1400–1403.Google Scholar

Shkuratov, Y., Starukhina, L., Hoffmann, H., & Arnold, G. (1999) A model of spectral albedo of particulate surfaces: Implications for optical properties of the Moon. Icarus, 137, 235–246.Google Scholar

Sunshine, J.M. & Pieters, C.M. (1993) Estimating modal abundances from the spectra of natural and laboratory pyroxene mixtures using the modified Gaussian model. Journal of Geophysical Research, 98, 9075–9087.Google Scholar

Sunshine, J.M., Bus, S.J., McCoy, T.J., Burbine, T.H., Corrigan, C.M., & Binzel, R.P. (2004) High‐calcium pyroxene as an indicator of igneous differentiation in asteroids and meteorites. Meteoritics and Planetary Science, 39, 1343–1357.Google Scholar

Sunshine, J.M., Farnham, T.L., Feaga, L.M., et al. (2009) Temporal and spatial variability of lunar hydration as observed by the Deep Impact spacecraft. Science, 326, 565–568.Google Scholar

Takir, D. & Emery, J.P. (2012) Outer main belt asteroids: Identification and distribution of four 3-μm spectral groups. Icarus, 219, 641–654.Google Scholar

Tholen, D.J. (1984) Asteroid taxonomy from cluster analysis of photometry. PhD thesis, University of Arizona, Tucson.Google Scholar

Thomas, C.A., Emery, J.P., Trilling, D.E., Delbó, M., Hora, J.L., & Mueller, M. (2014) Physical characterization of Warm Spitzer-observed near-Earth objects. Icarus, 228, 217–246.Google Scholar

Vernazza, P., Binzel, R., Thomas, C., et al. (2008) Compositional differences between meteorites and near-Earth asteroids. Nature, 454, 858–860.Google Scholar

Vernazza, P., Carry, B., Emery, J., et al. (2010) Mid-infrared spectral variability for compositionally similar asteroids: Implications for asteroid particle size distributions. Icarus, 207, 800–809.Google Scholar

Vernazza, P., Delbo, M., King, P., et al. (2012) High surface porosity as the origin of emissivity features in asteroid spectra. Icarus, 221, 1162–1172.Google Scholar

Vernazza, P., Castillo-Rogez, J., Beck, P., et al. (2017) Different origins or different evolutions? Decoding the spectral diversity among C-type asteroids. The Astronomical Journal, 153, 72.Google Scholar

Veverka, J., Thomas, P., Harch, A., et al. (1997) NEAR’s flyby of 253 Mathilde: Images of a C asteroid. Science, 278, 2109–2114.Google Scholar

Vilas, F. & Gaffey, M.J. (1989) Phyllosilicate absorption features in main-belt and outer-belt asteroid reflectance spectra. Science, 246, 790–792.Google Scholar

Walsh, K.J., Morbidelli, A., Raymond, S.N., O’Brien, D., & Mandell, A. (2012) Populating the asteroid belt from two parent source regions due to the migration of giant planets—“The Grand Tack.” Meteoritics and Planetary Science, 47, 1941–1947.Google Scholar

Weissman, P.R., A’Hearn, M.F., McFadden, L., & Rickman, H. (2002) Evolution of comets into asteroids. Asteroids III, 669–686.Google Scholar

Wenger, M., Ochsenbein, F., Egret, D., et al. (2000) The SIMBAD astronomical database-The CDS reference database for astronomical objects. Astronomy and Astrophysics Supplement Series, 143, 9–22.Google Scholar

Wigton, N.R. (2015) Near-infrared (2–4 micron) spectroscopy of near-Earth asteroids: A search for OH/H₂O on small planetary bodies. MS thesis, University of Tennessee.Google Scholar

Xu, S., Binzel, R.P., Burbine, T.H., & Bus, S.J. (1995) Small Main-Belt Asteroid Spectroscopic Survey: Initial results. Icarus, 115, 1–35.Google Scholar

Yang, B. & Jewitt, D. (2010) Identification of magnetite in B-type asteroids. The Astronomical Journal, 140, 692–698.Google Scholar

Zubko, E., Shkuratov, Y., Mishchenko, M., & Videen, G. (2008) Light scattering in a finite multi-particle system. Journal of Quantitative Spectroscopy and Radiative Transfer, 109, 2195–2206.Google Scholar

A’Hearn, M.F., Schleicher, D.G., Feldman, P.D., Millis, R.C. & Thompson, D.T. (1984) Comet Bowell 1980b. The Astronomical Journal, 89, 579–591.Google Scholar

Ammannito, E., De Sanctis, M.C., Capaccioni, F., et al. (2013a) Vestan lithologies mapped by the visual and infrared spectrometer on Dawn. Meteoritics and Planetary Science, 48, 2185–2198.Google Scholar

Ammannito, E., De Sanctis, M., Palomba, E., et al. (2013b) Olivine in an unexpected location on Vesta’s surface. Nature, 504, 122–125.Google Scholar

Ammannito, E., DeSanctis, M., Ciarniello, M., et al. (2016) Distribution of phyllosilicates on the surface of Ceres. Science, 353, aaf4279.Google Scholar

Barucci, M.A., Fulchignoni, M., & Rossi, A. (2007) Rosetta asteroid targets: 2867 Steins and 21 Lutetia. Space Science Reviews, 128, 67–78.Google Scholar

Barucci, M.A., Filacchione, G., Fornasier, S., et al. (2016) Detection of exposed H₂O ice on the nucleus of comet 67P/Churyumov-Gerasimenko-as observed by Rosetta OSIRIS and VIRTIS instruments. Astronomy and Astrophysics, 595, A102.Google Scholar

Binzel, R.P., Gaffey, M.J., Thomas, P.C., Zellner, B.H., Storrs, A.D., & Wells, E.N. (1997) Geologic mapping of Vesta from 1994 Hubble space telescope images. Icarus, 128, 95–103.Google Scholar

Birlan, M., Vernazza, P., Fulchignoni, M., et al. (2006) Near infra-red spectroscopy of the asteroid 21 Lutetia-I. New results of long-term campaign. Astronomy and Astrophysics, 454, 677–681.Google Scholar

Burbine, T.H., McCoy, T.J., Nittler, L.R., Benedix, G.K., Cloutis, E.A., & Dickinson, T.L. (2002) Spectra of extremely reduced assemblages: Implications for Mercury. Meteoritics and Planetary Science, 37, 1233–1244.Google Scholar

Capaccioni, F., Coradini, A., Filacchione, G., et al. (2015) The organic-rich surface of comet 67P/Churyumov-Gerasimenko as seen by VIRTIS/Rosetta. Science, 347, aaa0628.Google Scholar

Ciarniello, M., Capaccioni, F., Filacchione, G., et al. (2011) Hapke modeling of Rhea surface properties through Cassini-VIMS spectra. Icarus, 214, 541–555.Google Scholar